期刊名称：GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS
 期刊简介(About the journal)
投稿须知(Instructions to Authors)
编辑部信息(Editorial Board)
About the journal
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Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects.
In addition, their magnetohydrodynamic behaviors are investigated. Experimental, theoretical and numerical studies of rotating, stratified and converging fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.
The current impact factor is 0.881
Abstracting Information:
Geophysical and Astrophysical Fluid Dynamics is abstracted in Elsevier Geo Abstracts; Mathematical Reviews; Meteorlogical / Geo Abstracts; ISI Cambridge Scientific Abstracts; New Jour; ISI Current Contents: Physical, Chemical & Earth Sciences; Astrophysics Data System and SciBase. |
Instructions to Authors
Manuscripts. All submissions will be subject to the normal process of peer review. Please submit three copies of your manuscript, typed on one side of the paper and double spaced, as well as an electronic version on disk (see below) to the Editor or the appropriate Associate Editor (see inside front cover). Contributors should note that material submitted to the journal must be original, must not have already appeared in another publication and
must not be submitted for publication elsewhere while under consideration by the journal.
The title of the paper and the author(s) name(s) should appear at the beginning of the paper. All pages of the manuscript must be numbered. All manuscripts should include full correspondence details (street address, telephone, fax and email addresses) of the corresponding author. The paper should also include an abstract (of 100–150 words)
and 3–6 keywords. The language of publication is English and US spelling is preferred.
Please make sure your contact address infor-mation is clearly visible on the outside of all
packages you are sending to Editors.
Disk submissions. Authors should send the final, revised version of their article in both hard copy (paper) and electronic (disk) forms. It is essential that the hard copy (paper) version exactly matches the material on disk. Please print out the hard copy from the disk you are sending. Submit three printed copies of the final version with the disk to the Editor
who is handling your paper. Save all files on a standard 3.5-inch high-density disk. We prefer to receive disks in Microsoft Word (PC format), TeX or LaTeX format, but can translate from most other common word-processing programs as well as Macs. Please specify which program you have used. Do not save your files as ‘‘text only’’ or ‘‘read
only’’.
Tables and figures. Tables must be typed on separate sheets and not included as part of the text. The captions to illustrations should be gathered and typed on a separate sheet. Tables should be numbered by Roman numerals and figures by Arabic numerals. The approximate position of tables and figures should be indicated in the paper. Please supply clear copies of artwork (preferably the originals) for figures in a finished format suitable for reproduction. Photographs intended for halftone reproduction must be good glossy original prints, of maximum contrast. Clearly label each figure with author’s name and figure number, indicating ‘‘top’’ where this is not obvious.
Figures will not normally be redrawn by the publisher. The author(s) must arrange permission for the reproduction of illustrations and tables within articles. Figures may be sent electronically, pre-ferably in either TIFF (tagged image format) or EPS
(encapsulated Postscript) formats. However, we can also accept PICT or JPEG formats. The publisher will normally reproduce colour figures in black and white.
Mathematical expressions and equations In the text avoid superscripted and subscripted expres-sions (e.g. Instead of e i kx and 3 4 write exp ð i kx Þ and 3 =4 ). In the displayed equations, avoid both over congestion and unnecessary empty spaces; aim for clarity and compactness. Algebraic letters should generally be italic; the exceptions, which are roman, are functions (e.g. sin ), e and i as in e i kx , and the differential d as in d r =d t and R v d t . Vectors are bold roman and the gradient operator is bold (e.g.F ¼ J¼ñêôœ`), except for its scalar use (e.g. r 2 u ).
The ‘dot’ in the scalar product is bold (e.g. x u and J u ), as is the ‘times’ in ther vector product (e.g. j B and J B ).
References These should be indicated in the text by the Harvard (name and date) system. The full list of references should be collected at the end of the paper in alphabetical order and should be complete in all details. Article titles should be enclosed in quotation marks and abbreviation of journal titles should follow Physical Abstracts style. The initials
of the authors should be placed after their names and the year of publication placed in parentheses at the end of the reference. Examples: McWiliams, J.C. and Flierl, G.R., ‘‘On the evolution of isolated nonlinear vortices’’, J. Phys. Oceanogr. 9, 1155–1182 (1979).
Schubert, G., Turcote, D.L. and Olson, P., Mantle Convection in the Earth and Planets, Cambridge University Press (2001).
Roberts, P.H., ‘‘Fundamentals of dynamo theory’’. In: Lectures on Solar and Planetary Dynamos (Eds. M.R.E. Proctor and A.D. Gilbert) pp. 1–58, Cam-bridge University Press (1994).
Early Electronic Offprints: Corresponding authors can now receive their article by e-mail as a complete PDF. This allows the author to print up to 50 copies, free of charge, and disseminate them to colleagues. In many cases this facility will be available up to two
weeks prior to publication. Or, alternatively, corre-sponding authors will receive the traditional 50 offprints. A copy of the journal will be sent by post to all corresponding authors after publication. Addi-tional copies of the journal can be purchased at the
author’s preferential rate of £15.00 per copy. Copyright. It is a condition that authors vest
copyright in their articles, including abstracts, in Taylor & Francis Ltd. This enables us to ensure full copyright protection and to disseminate the article, and the journal, to the widest possible readership in print and electronic formats as appropriate. Authors may use their article elsewhere after publication provided that prior permission is obtained from Taylor & Francis Ltd. Authors are themselvesresponsible for obtaining permission to reproduce copyright material from other sources.
Editorial Board
Editor:
Professor A. M. Soward,School of Mathematical Sciences, University of Exeter, Laver Building, North Park Road, Exeter EX4 4QE, UK
Associate Editors:
F. H. Busse - Institute of Physics, University of Bayreuth, D-95440 Bayreuth, Germany
G. A. Glatzmaier - Earth Sciences Department, Marine Sciences Building, University of California, Santa Cruz, CA 95064, USA
W. R. Peltier - Department of Physics, University of Toronto, 215 Huron Street, Toronto, Ontario M5S 1A1, Canada
J. A. Whitehead - Department of Physical Oceanography, Woods Hole Oceanographic Institution, Mail Stop #21, Woods Hole, Massachusetts 02543-1047, USA
T. Yamagata - Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo, 7-3-1 Hong, Bunkyo-ku, Tokyo 113-0033, Japan
Editorial Board:
S. I. Braginsky - Institute of Geophysics and Planetary Physics (IGPP), University of California (UCLA), USA
S. M. Chitre - Theoretical Astrophysics Group, Tata Institute of Fundamental Research, India
P. A. Davies - Department of Civil Engineering, The University of Dundee, UK
U. Frisch - Observatoire de la Côte d’Azur, France
G. S. Golitsyn - Institute of Atmospheric Physics, Academy of Sciences, Russia
R. H. J. Grimshaw - Department of Mathematical Sciences, Loughborough University, UK
P. Hejda - Deputy Director, Geophysical Institute, Czech Republic
G. J. F. van Heijst - Fluid Dynamics Laboratory, Eindhoven University of Technology, The Netherlands
R. Hide - Department of Mathematics, Imperial College London, UK
J. A. Johnson - School of Mathematics, University of East Anglia, UK
C. A. Jones - School of Mathematical Sciences, University of Exeter, UK
M. Kono - Institute for Study of the Earth's Interior, Okayama University, Japan
A. Majda - Courant Institute of Mathematical Sciences, New York University, USA
J. C. McWilliams - Institute of Geophysics and Planetary Physics (IGPP), University of California (UCLA), USA
E. N. Parker - Illinois, USA
E. R. Priest - Department of Mathematical Sciences, University of St Andrews, UK
M. R. E. Proctor - Department of Applied Mathematics and Theoretical Physics, Cambridge University, UK
P. H. Roberts - Mathematics Department, University of California (UCLA), USA
G. Rudiger - Astrophysikalisches Institut Potsdam, Germany
A. A. Ruzmaikin - Jet Propulsion Laboratory (JPL), California Institute of Technology, USA
R. Salmon - Physical Oceanography Building, Scripps Institution of Oceanography, USA
D. Sokoloff - Department of Physics, Moscow State University, Russia
E. A. Spiegel - Department of Physics and Astronomy, Columbia University, USA
H. Yosimura - Department of Astronomy, University of Tokyo, Japan
E. G. Zweibel - Department of Astronomy, University of Wisconsin, USA
Book Review Editor: A. D. Gilbert - School of Mathematical Sciences, University of Exeter, UK
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